Earthquake fault dynamics: Insights from laboratory experiments

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Friction controls earthquake physics. No direct access to the “earthquake engine”. Earthquake simulation in the lab: friction machines. Examples of experiments ...
Earthquake fault dynamics: Insights from laboratory experiments INGV

S. Nielsen

G. Di Toro, A. Niemeijer, E. Spagnuolo, M. Violay, S. Smith, N. De Paola, A. Bistacchi, G. Pennacchioni, F. Di Felice, G. Romeo, R. Han, T. Hirose, K. Mizoguchi, M. Cocco, T. Shimamoto.

This research is funded by the European Research Council

Acknowledgements S. Nielsen (1) G. Di Toro (1, 2) A. Niemeijer (1, 4), E. Spagnuolo (1), M. Violay (1), S. Smith (1), N. De Paola (5), A. Bistacchi (6), G. Pennacchioni (2), F. Di Felice (1), G. Romeo (1), R. Han (7), T. Hirose (7), K. Mizoguchi (7), M. Cocco (1), T. Shimamoto (3), ...

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(2)

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INGV Geoscienze, Uni. Padova

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This research is funded by the European Research Council

Earthquakes are caused by fracture and frictional slip on faults. Friction is a key parameter in understanding the physics seismic source. Let's investigate friction under Earth crust conditions.

Fault surface in dolomite, Southern Alps, Italy

Arrest or propagation of dynamic rupture

Friction law Energy balance: dissipation, heat, seismic radiation

Rupture velocity Slip velocity, rise time

Friction and energy peak

recovery

decay steady-state

L'AQUILA Courtesy of: Stefano Pucci, INGV

TOHOKU Courtesy of: Singapore Earthquake Observatory and USGS

20 km

No direct access to the “earthquake engine”...

Let's try to re-create it in the lab?

Synopsis Friction controls earthquake physics No direct access to the “earthquake engine” Earthquake simulation in the lab: friction machines Examples of experiments and typical results Lubrication processes and rock types Extrapolating the results: faults are weak during earthquakes Conclusions and future research

Experimental machines LOW STRAIN (old-style shear or rotary) HVRF (High-velocity, Rotary Shear machines) SHIVA (Slow to HIgh Velocity Apparatus) Experimental machines are NOT designed to predict earthquakes!! They help our understanding of earthquake physics and thus improve modeling and risk assessment.

µ = τ / σn Shear stress, GPa

e y “B

s ’ e rle

” w la

1.0

0.5

Low friction during EQs? 0.5

1

1.5

2.0

Normal stress, GPa [Byerlee, PAGEOPH,1978]

Rate and State

µ A

B Dc

V=0.4 mm/s V= 4 mm/s

µ friction coeff. A & B constants Dc critical slip 10-6-10-4 m θ (s) state variable V slip rate - s slip

[from Marone, 1998]

friction drop is small velocity dependance is small stress and velocity cover only part of seismic faulting conditions

The principle of ROTARY machines

Rotating shaft

HOLDERS

(torque act.)

PAIR OF CYLINDRICAL SAMPLES

Axial shaft (normal load act.)

Experimental conditions “Traditional” machines SHIVA still out of reach...

Experimental conditions and earthquake conditions

Shallow “Typical” earthquakes crustal earthquakes

Deep earthquakes

Machine “1”, Kyoto Univ., Japan, ca. 1990 (T. Shimamoto)

NIED 2007 Designed by Mizoguchi

σ n < 20 MPa v = 0.1 µm/s - 10 m/s d = infinite

SHIVA, Italy, Sept 2009 (designed by an Italian Team at INGV) σ n < 50 MPa v = 1 µm/s - 9 m/s d = infinite Seismic accelerations

1m

SHIVA, Italy, Sept 2011 INGV

1

3

2a

2b

SERVO-CONTROL 200kW drive

Video examples of the experimental dynamics

Dry, slicatic rocks --> melting

Natural faults Lab

MYLONITE (Maine)

SILTSTONE

METAGABBRO (Premosello-Italian Alps)

What do we measure?

FRICTIONAL resistance of the sample while it is sliding SHORTENING of the sample under the effect of frictional wear GAS EMISSIONS during the sliding TEMPERATURES in or around the sample close to the slip surface SLIDING VELOCITY is retrieved from rotative motion and sample radius

Example:

Synopsis Friction controls earthquake physics No direct access to the “earthquake engine” Earthquake simulation in the lab: friction machines Examples of experiments and typical results Lubrication processes and rock types Extrapolating the results: faults are weak during earthquakes Conclusions and future research

High velocity friction; lubrication

Large slip & slip-rate Intermediate normal stress Considerable WEAKENING

Lubrication effect Byerlee friction H-V friction

Nielsen et al., 2008  

 

After Di Toro et al., 2005

The key is high work rate generating heat density

Heat density

Temperature increase

Specific heat of water, evaporation, fluid pressurization

Latent heat of chemical processes and phase transitions (decarbonation, gelification, dehydration, serpentinization, poorly known tribolchemical processes...)

Dynamic fault slip, heat and friction:

 Large, fast slip means concentrated heat  Heat triggers a variety of weakening mechanisms  Under favourable conditions melt is produced

In its most straightforward manifestation, elevated heat density induces temperature rise and eventually yields to melting... But not always! ( maybe even seldom )

Observed processes in HV rock friction: Silica gel lubrication (quartz rocks) Thermal decomposition and nanopowders (limestones) Thermal decomposition and pressurization (dolostones) Clay-gouge weakening, dehydration and press. (clay-gouges) Flash heating (small slip amounts) Melt lubrication (all silicate built rocks)

A very inclomplete classification of rock types and frictional processes Cohesive Silicatic

Melting Silica gel lubrication Flash heating Dehydration

Carbonatic

Decarbonation Plastic yielding Dehydration Flash heating Nanopowder lub.

Non-cohesive & clays

Flash heating Decarbonation Nanopowder lub.

For most process and rock types lubrication is observed at high velocity

Not much weakening..

Friction Di Toro et al., in preparation

Seismic slip rates

Significant weakening around 0.1 m/s Different rock types (carbonates, silicates, ...)

Friction Di Toro et al., in preparation

Seismic slip rates

Work rate or power density

Friction Di Toro et al., in preparation

Cohesive Rocks: desaggregation in the results for various compositions suggest different thermal activation mechanisms.

I AT ON RB CA DE

GE LI F ICA TIO N

MELTING ON

with gouge - Brantut et al., 2008 Fault zone rich in kaolinite dehydratation at ~1m/s, ~1 MPa

Clay-clast aggregates (FE-SEM image)

(e.g., Bouteraud et al., 2008)

MELTING: glass and survivor clasts (SEM image)

pyroxene with embayment

vesicles

glass feldspar clast

20 µm

Synopsis Friction controls earthquake physics No direct access to the “earthquake engine” Earthquake simulation in the lab: friction machines Examples of experiments and typical results Lubrication processes and rock types Extrapolating the results: faults are weak during earthquakes Conclusions and future research

Extrapolation How to upscale lab to EQ conditions? Larger σn,V, accelerations Larger size than sample Complex slip time-history Complex geometry Different petrology/chemestry Different fabric

Extrapolation

I SEISMICITY, statistics of a fault population, correlations, criticality....: the process from a global point of view – YESTERDAYS TOPIC

III II LAB: small portion of a fault - scale 2 - 5 cm

SISMO: “global” rheology of the whole fault

Conclusions No direct access to the “earthquake engine” Earthquake simulation in the lab: friction machines High POWER (hich slip vel. and normal load combined) yields lubrication Various lubrication processes depending on rock types Extrapolating the results: power laws and geometry problems We barely start to measure and understand...

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